@inproceedings{62ce503d52be4960bdde4664b2d3c62f,
title = "Solar system studies with the Arecibo planetary radar system",
abstract = "The 305 m Arecibo telescope equipped with a 1 MW 2.38 GHz transmitter is used for studies of the terrestrial planets, planetary satellites including the Moon and small bodies in the solar system. Much of the recent program emphasis has been on astrometric and characterization observations of near-Earth objects for which the Arecibo radar system has capabilities not matched by any other Earth-based telescope. However, studies of the surfaces of Mercury, the Moon and Mars continue and renewed observations of Venus are planned.",
author = "Campbell, \{Donald B.\} and Harmon, \{John K.\} and Nolan, \{Michael C.\}",
year = "2011",
doi = "10.1109/URSIGASS.2011.6051217",
language = "English (US)",
isbn = "9781424451173",
series = "2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011",
booktitle = "2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011",
note = "2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011 ; Conference date: 13-08-2011 Through 20-08-2011",
}